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This work evaluates differential sensitivity in gamma rays detection, focusing on Imaging Atmospheric Cherenkov Telescopes for astrophysical observations.
This work is devoted to the evaluation of the differential sensitivity of the 5 Imaging Atmospheric Cherenkov Telescopes (IACTs) under construction as part of the TAIGA astrophysical complex. The procedure for simulating detected gamma rays with energies from 2 to 200 TeV in the stereo mode of observations is described, along with the procedure of gamma–hadron separation for determining the differential sensitivity of the facility.
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Волчугов et al. (2025) studied this question.
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